The Astrophysical Journal Supplement Series 212, 27 May 2014 [Refereed]
We propose the application of coronagraphic techniques to the spectroscopic
direct detection of exoplanets via the Doppler shift of planetary molecular
lines. Even for an unresolved close-in planetary system, we show that the
combination of a visi...
Astrophysical Journal 758(1) 13 Oct 2012 [Refereed]
The oxygen absorption line imprinted in the scattered light from the Earth- like planets has been considered the most promising metabolic biomarker of the exo-life. We examine the feasibility of the detection of the 1.27 μm oxygen band from habita...
We perform a systematic X-ray analysis of six giant radio relics of four
clusters with Suzaku satellite by compiling new analysis of CIZA 2242.8-5301,
Zwcl 2341.1-0000, and Abell 3667 and previous results of A3667 and A3376.
Especially we first ob...
Aiming at obtaining detailed information of surface environment of
Earth-analogs, Kawahara & Fujii 2011 proposed an inversion technique of annual
scattered light curves named the spin-orbit tomography (SOT), which enables one
to sketch a 2-dimensi...
Mark Swain, Pieter Deroo, Giovanna Tinetti, Morgan Hollis, Marcell Tessenyi, Michael Line, Hajime Kawahara, Yuka Fujii, Adam Showman, Sergey Yurchenko
We report near-infrared measurements of the terminator region transmission
spectrum and dayside emission spectrum of the exoplanet WASP-12b obtained using
the HST WFC3 instrument. The disk-average dayside brightness temperature
averages about 2900...
We develop an inversion technique of annual scattered light curves to sketch a two-dimensional albedo map of exoplanets in face-on orbits. As a test bed for future observations of extrasolar terrestrial planets, we apply this mapping technique to ...
Yuka Fujii, Hajime Kawahara, Yasushi Suto, Satoru Fukuda, Teruyuki Nakajima, Timothy A. Livengood, Edwin L. Turner
ApJ 738 184 Aug 2011 [Refereed]
As a test-bed for future investigations of directly imaged terrestrial
exoplanets, we present the recovery of the surface components of the Earth from
multi-band diurnal light curves obtained with the EPOXI spacecraft. We find
that the presence an...
Yoh Takei, Eugenio Ursino, Enzo Branchini, Takaya Ohashi, Hajime Kawahara, Kazuhisa Mitsuda, Luigi Piro, Alessandra Corsi, Lorenzo Amati, Jan-Willem den Herder, Massimiliano Galeazzi, Jelle Kaastra, Lauro Moscardini, Fabrizio Nicastro, Frits Paerels, Mauro Roncarelli, Matteo Viel
ApJ 734(2) 91 Jun 2011 [Refereed]
We assess the possibility to detect the warm-hot intergalactic medium (WHIM)
in emission and to characterize its physical conditions and spatial
distribution through spatially resolved X-ray spectroscopy, in the framework of
the recently proposed ...
The recently introduced discrete persistent structure extractor (DisPerSE,
Soubie 2010, paper I) is implemented on realistic 3D cosmological simulations
and observed redshift catalogues (SDSS); it is found that DisPerSE traces
equally well the obs...
We report on a new merging group of galaxies, Suzaku J1552+2739 at z ~ 0.08
revealed by a SUZAKU observation. The group was found by observing a junction
of galaxy filaments optically identified in the Sloan Digital Sky Survey
spectroscopic data. ...
Scattered lights from terrestrial exoplanets provide valuable information
about the planetary surface. Applying the surface reconstruction method
proposed by Fujii et al. (2010) to both diurnal and annual variations of the
scattered light, we deve...
Erik D. Reese, Hajime Kawahara, Tetsu Kitayama, Naomi Ota, Shin Sasaki, Yasushi Suto
ApJ 721(1,Pt.1) 653-669 Aug 2010 [Refereed]
We perform a uniform, systematic analysis of a sample of 38 X-ray galaxy
clusters with three different Chandra calibrations. The temperatures change
systematically between calibrations. Cluster temperatures change on average by
roughly ~6% for the...
We derive the axis ratio distribution of X-ray clusters using the XMM-Newton
catalogue (Snowden et al. 2008). By fitting the contour lines of the X-ray
image by ellipses, we confirm the X-ray distribution is well approximated by
the elliptic distr...
Y. Fujii, H. Kawahara, Y. Suto, A. Taruya, S. Fukuda, T. Nakajima, E. L. Turner
ApJ 715(2,Pt.1) 866-880 Jun 2010 [Refereed]
Characterizing the surfaces of rocky exoplanets via the scattered light will
be an essential challenge to investigate the existence of life on habitable
exoplanets. We present a simple reconstruction method for fractional areas of
Hajime Kawahara, Erik D. Reese, Tetsu Kitayama, Shin Sasaki, Yasushi Suto
ApJ 687(2) 936-950 Nov 2008 [Refereed]
Our previous analysis indicates that small-scale fluctuations in the
intracluster medium (ICM) from cosmological hydrodynamic simulations follow the
lognormal distribution. In order to test the lognormal nature of the ICM
directly against X-ray ob...
The Hubble constant estimated from the combined analysis of the
Sunyaev-Zel'dovich effect and X-ray observations of galaxy clusters is
systematically lower than those from other methods by 10-15 percent. We examine
the origin of the systematic und...
We carried out observations of the central and 20' east offset regions of the
cluster of galaxies Abell 1060 with Suzaku. Spatially resolved X-ray spectral
analysis has revealed temperature and abundance profiles of Abell 1060 out to
27' ~ 380; /h...